3D self-consistent continuum radiative transfer code based on the Monte-Carlo Method

3D self-consistent N-body barred models of the Milky Way: I. Stellar dynamics

3D self-consistent N-body barred models of the Milky Way: II. Gas dynamics

3D Semiconductor Detectors For New Focusing Hard X And Soft Gamma-ray Telescopes

3D Simulation of Convection and Spectral Line Formation in A-type Stars

3D simulation of flux emergence from convective zone to corona with BATSRUS

3D Simulation of the Gas Dynamics in the Central Parsec of the Galaxy

3D simulations identifying the effects of varying the twist and field strength of an emerging flux tube

3D Simulations of Betelgeuse's Bow Shock

3D simulations of Einstein's equations: symmetric hyperbolicity, live gauges and dynamic control of the constraints

3D Simulations of Fluctuation Spectra in the Hall-MHD Plasma

3D Simulations of Galactic Winds in Dwarf Galaxies

3D simulations of gyrosynchrotron emission from mildly anisotropic nonuniform electron distributions in symmetric magnetic loops

3D simulations of linearized scalar fields in Kerr spacetime

3D simulations of M star atmosphere velocities and their influence on molecular FeH lines

3D Simulations of Magnetic Massive Star Winds

3D Simulations of Magnetohydrodynamic Waves in the Magnetized Solar Atmosphere

3D Simulations of MHD Jet Propagation Through Uniform and Stratified External Environments

3D simulations of microquasar jets in clumpy stellar winds

3D simulations of pillars formation around HII regions: the importance of shock curvature